Power-spectrum analysis of preflare solar X rays

Astronomy and Astrophysics – Astronomy

Scientific paper

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Power Spectra, Solar Flares, Solar Spectra, Solar X-Rays, Fourier Transformation, H Alpha Line, Spectrum Analysis

Scientific paper

A spectral analysis of the data obtained from the Prognoz 5 - 7 stations in the course of the experiment on the measurement of solar soft X-rays before hard X-ray bursts has been carried out (Kocharov et al., 1983). Several quasi-periodic components (with periods ≡1.5 hour, ≡40, ≡10, ≡2 min) have been found, and time variations of their parameters while approaching the burst have been studied. These components may serve as one of the indications of a pre-flare situation.

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